Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Institute of Geophysics and Planetary Physics, University of California, Riverside, CA 92521 of Geophysics and Planetary Physics, University of California, Riverside, CA 92521; On leave from the Institute for Problems in Mechanics, Russian Academy of Sciences, Vernadskii Avenue 101-1, Moscow 119526, Russia. of Geophysics and Planetary Physics, University of California, Riverside, CA 92521
Institute of Geophysics and Planetary Physics, University of California at Riverside, 900 University Avenue, Riverside, CA 92521
Institute for Problems in Mechanics, Russian Academy of Sciences, Moscow, Russia
Physics Department and Center for Space Plasma and Aeronomic Research, The University of Alabama in Huntsville, 320 Sparkman Dr., Huntsville, AL 35805, USA of Geophysics and Planetary Physics, University of California, Riverside, CA 92521 of Geophysics and Planetary Physics, University of California at Riverside, 900 University Avenue, Riverside, CA 92521 University of Alabama in Huntsville, CSPAR, Huntsville, AL 35805, USA; Also at Physics Department, The University of Alabama in Huntsville, Huntsville, AL 35805, USA
Center for Space Plasma and Aeronomic Research, University of Alabama in Huntsville, Huntsville, AL 35805, USA ; Department of Physics, University of Alabama in Huntsville, Huntsville, AL 35899, USA
Russian Academy of Sciences, Inst. for Problems in Mechanics
The University of Alabama in Huntsville, Physics Department / CSPAR, NSSTC Bld., 320 Sparkman Drive, Huntsville, AL 35805, USA
Institute for Problems in Mechanics, Russian Academy of Sciences 101-1 Vernadskii Avenue, Moscow 117526, Russia of Geophysics and Planetary Physics, University of California, Riverside, CA 92521 Department and Center for Space Physics and Aeronomic Research, The University of A
3D Heliospheric Simulations of Heavy Neutral Particles from the Interstellar Medium
5th International Conference of Numerical Modeling of Space Plasma Flows (ASTRONUM 2010)
A New, Three-dimensional, Adaptive Mesh Refinement Code for Modeling Flows of Partially Ionized Plasma
Absorption signatures of the heliosphere
Accretion Flows: Aspects of Gas Dynamic Modeling
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